A solar panel, and the sign integration grew
Point a solar panel straight at the sun and it harvests the most power it can. Tilt it and the yield falls off. Turn it edge-on — its face parallel to the incoming light — and it collects nothing, even though the sun is blazing at full strength. The power a panel collects is the field of sunlight dotted with the panel's normal direction: , and that dot product falls as as you tilt.
The same dot product is how 3-D graphics decides how bright a surface looks — Lambert shading is between a light direction and a surface normal, the exact computation in the renderers behind every game and animated film. This chapter is the calculus of that idea: integrating a quantity over a curved surface, and the orientation choice that gives the answer its sign.
A surface integral totals something spread over a curved sheet — its area, its mass, or the flux of a field through it (how much flows across). And just as Chapter 13's Green's theorem traded a boundary loop for the region inside, Stokes' theorem trades a loop in 3-D space for a flux through any surface that loop bounds. One honest warning up front: nobody pictures a curved surface whole. We parametrise it down to a flat rectangle and integrate there — the 3-D version of Chapter 10's shadow-and-slice.
Parametrising a surface, and the element
The five-step spine you have run since Chapter 10 does not change — only two of its steps swap out. A solid was described by sketch → shadow → slice. A surface is described by parametrise → build the normal → orient:
| 1 | 2 | 3 | 4 | 5 | |
|---|---|---|---|---|---|
| Solids (Ch 10–13) | sketch | shadow | slice | limits | integrate |
| Surfaces (Ch 14) | parametrise | ru × rv | orient | (u,v) limits | integrate |
Three steps keep their role (draw/describe, read the limits, integrate). The two solid-only steps — shadow and slice — swap for the two surface-only steps: build the normal with a cross product, and orient it. "Orient" is a named guardrail, because orientation is exactly where marks leak.
A surface is a map from a flat domain . The two tangent vectors and span the little patch, and their cross product does triple duty:
- It is perpendicular to the surface — so it is the normal direction.
- Its length is the area of the little parallelogram the patch spans — so is exactly per unit . (It is the Jacobian of the surface map — the same area-scaling machine as Chapters 11 and 12, now mapping a flat rectangle onto a curved sheet.)
- Its direction is the normal that carries the orientation — the sign of the flux.
The graph case is the most common exam surface, and there the domain is the -shadow of the surface — the one place the old word "shadow" still applies literally.
Find the surface area of a sphere of radius using . The cross product of the tangent vectors works out to
The element is the spherical surface Jacobian — the same that ran through Chapter 12's volume element, now without the . The machine recovers the area you already trust; a hemisphere () gives .
Scalar surface integrals
With in hand, a scalar surface integral is just "sum over the sheet":
Take and you get area; density and you get the mass of a curved sheet (a dome, a shell, a sail); divide by area and you get an average value. There is no orientation here — a scalar integral uses the length , which is always positive.
Evaluate over the upper hemisphere , . On the sphere and , with :
The same you met computing the hemisphere's centroid in Chapter 12 — the machinery is genuinely shared across the unit.
End of sitting 1 — you can parametrise a surface, build from the cross product (and the graph shortcut ), and integrate a scalar over it. After the break: flux and the orientation sign that trips everyone, then Stokes' theorem — Green's theorem lifted off the plane — with two playgrounds to drill both.
Flux, and the sign that follows your choice
Flux measures how much of a field crosses a surface. It is the field dotted with the normal, summed over the sheet — and because the normal keeps its direction this time, the vector cross product is used, sign and all:
A surface has two normals — the patch can face either way — and choosing one is choosing the sign. "Outward" (for a closed surface) and "upward" (for a graph) are the usual conventions, but the problem statement decides. The flux sign follows the normal you pick — this is the chapter's headline error.
Find the flux of through the paraboloid cap , . As a graph, the upward normal vector is , so on the surface . Polar over the unit-disk shadow:
Identical surface, identical field — the only difference is which way points, and that flips the sign. Quote a flux without stating the orientation and the number is only half an answer.
Playground 1 — Flux Tilt
A flat panel of area sits in a uniform field of strength . Drag the panel's tilt and toggle which way its normal points, then — before you reveal — predict the sign of the flux. Watch it vanish edge-on, and flip when you flip the normal.
Edge-on (θ = 90°) the flux is 0 in every preset — the field grazes the panel and nothing crosses, though the field is at full strength. The minus normal flips the sign; θ = 0° gives the maximum ±F₀·A.
Stokes' theorem
In 3-D the curl becomes a vector — it measures the axis and rate of a field's local spinning:
Chapter 13's flat scalar curl was just the -component of this — the part that spins in the plane. Stokes' theorem then says:
In words: a field's circulation around a closed space curve equals the flux of its curl through any surface that the curve bounds, with oriented by the right-hand rule about . Flatten everything to the plane () and this is Green's theorem from Chapter 13. Stokes is Green lifted off the plane.
Take , so , and let be the unit circle in the -plane, counterclockwise.
(the Chapter 13 area form).
(b) Stokes via the flat disk: ✓
Same rim, outward normal: ✓
Same value — the bulging dome and the flat disk agree.
The curl-flux did not care which surface you stretched across the loop — only the boundary. It is the same lesson as Chapter 13's "the integral sees only what the contour encloses," now one dimension up.
Playground 2 — Stokes Verifier
The field is fixed at . Pick a surface stretched across a rim, predict its curl-flux, and reveal it next to the boundary circulation . Swap to a different surface on the same rim — the value does not budge. Only changing the rim changes it.
All four unit-rim surfaces return 2π; the radius-2 surfaces return 8π. The value tracks the rim, never the surface — that is surface independence, the heart of Stokes.
Test yourself before moving on
Commit before reading the feedback. Two of these turn on the orientation sign — the exact place marks leak — on purpose.
Using a parametrisation, the surface area of a sphere of radius is:
The flux of through the paraboloid cap , , oriented downward, is:
For and the unit circle CCW, Stokes' theorem gives
is a messy closed loop in the -plane (awkward to parametrise) bounding a region of known area. To find for , the efficient route is:
The same , but with the unit circle taken clockwise (seen from ):
Exam translator — what a surface/Stokes question actually asks
In standard Indian engineering-math exams, and likely in MCC201A unless your class notes differ, this material asks four things:
- "Set up / evaluate " → parametrise, build (or for a graph), integrate over (WE1, WE2).
- "Find the flux of through (oriented …)" → use the vector ; the sign follows the stated orientation (WE3). This is where marks leak.
- "Verify Stokes' theorem for …" → compute both the loop integral and the curl-flux and show they match (WE4).
- "Using Stokes', evaluate …" → turn a hard loop integral into an easy curl-flux, or vice versa (Q4).
Worked solutions are complete; nothing points off this page. Do them as listed — interleaved on purpose. PR7 opens with a faded bridge: part of the work is set out, the key step left for you.
PR1 · surface area of a cone (graph)
PR1. Find the area of the cone below .
For , , so the factor is — constant. The shadow is the unit disk:
PR2 · scalar integral over that cone
PR2. Evaluate over that cone, .
On the cone and :
PR3 · flux through a cylinder side (both orientations)
PR3. Find the flux of through the side of the cylinder , , oriented outward.
Parametrise ; the outward normal is , so on the side , and :
Inward orientation flips it to . (The flat top and bottom caps are not part of "the side.")
PR4 · Stokes, where the sign rides the field
PR4. For and the unit circle CCW, find .
. The curl-flux through the disk is . Here the sign comes from the field (the curl points down), not from the orientation — contrast Q5, where the field was and the sign came from walking backwards.
PR5 · flux through a flat disk (orientation)
PR5. Find the flux of through the disk in the plane , oriented downward.
The disk has area . With the upward normal, , giving . Oriented downward, the sign flips:
PR6 · decision-only · which tool, and the value
PR6. bounds a region of area . For , name the efficient tool and give .
Stokes / Green. is constant, so the circulation — no parametrisation needed.
PR7 · faded bridge · surface independence, confirmed
PR7. For , confirm surface independence by computing over both the flat disk and the paraboloid cap (both with the unit-circle rim).
Bridge: . For the disk ; for the paraboloid the upward . Predict the next step: what is , and why does the integral come out the same?
Disk: , so . Paraboloid: as well — the curl's components are zero, so only the -part survives, and the integrand is again over the unit disk:
The curl had no sideways component, so the surface's bulge contributed nothing — only the rim mattered. That is surface independence in one line.
Three things to carry out of this chapter
- Parametrise, then the cross product does everything. is the area element (the surface Jacobian); its direction is the normal. Graphs get the shortcut .
- Flux carries a sign, and the sign is your choice of normal. Scalar integrals use the magnitude; flux keeps the vector. State the orientation or the answer is half done.
- Stokes is Green lifted off the plane: , and the curl-flux depends only on the boundary — any surface with the same rim gives the same value.
Back to the solar panel: the power it harvests is summed over its face — a flux integral — and edge-on it collects nothing, the same that opened the chapter. Orientation is not a technicality; it is the difference between a panel that works and one that doesn't. Re-do PR3 and PR7 from a blank page tomorrow — not re-read, re-do. Keeping the normal's direction straight is the muscle this chapter builds.
What's next. Chapter 15 closes the course with the divergence theorem — flux out through a closed surface equals the divergence summed over the solid inside — and then steps back to see Green's, Stokes', and Gauss's theorems as three faces of one idea: the boundary remembers the inside.
Same material, another voice
If a different explanation would help, this maps onto the chapter — free, from MIT OpenCourseWare:
- Read / watch: MIT 18.02SC — Part C: Line Integrals and Stokes' Theorem — frames Stokes as the extension of Green's, with the curl-flux over any surface sharing the boundary (exactly WE4 and the Stokes Verifier).
✓ Chapter complete. Your progress, and every quiz answer, is saved on this computer — revisit any time.